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Fig. 13

image

Normalized profile of the C i, C i, and C i lines near 1276 (top panel) and 1280 Å (bottom) at zabs ≃ 2.418 towards J1439+1117, seen on the Lyα emission line of this quasar. Observed profiles are shown in black, while the profiles derived from fitting of the 1560 and 1656 Å transitions observed against the continuum source are displayed in green and the profiles computed towards the ELR alone (see text) in red. C i absorption is significantly stronger towards the ELR for the three central components (at v = −10,0 and + 12 km s-1) as well as the C i absorption in the v = −10 km s-1 component. The velocity scale is the same as in Fig. 12.

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